It has mentioned that the gravitational waves emitted from the final stages of an inspiraling binary neutron star system are one of the most important sources for the terrestrial gravitational waves detectors [1]}, [2]}, [3]}, [4]}, [5]}, [6]}, [7]}, [8]}, [9]}. In such case, properties like the mass of the component stars can be measured. As Flanagan and Hinderer [3]} articulated, the tidal effects can be measurable during this final stage of the inspiral.
